Archival Hubble Images Reveal Neptune's “Lost” Inner Moon

Neptune's innermost moon, Naiad, is clearly seen here for the first time since the Voyager 2 flyby of 1989. The Hubble Space Telescope captured the tiny point of light just off to the side of Neptune in December, 2004. The detection went unnoticed until recently, when the images were re-analyzed using newly developed processing techniques. The new analysis employed special processing to suppress the extensive glare around Neptune, which is more than one million times brighter than the nearly 100-km object shown. The image is composed of eight four-minute exposures, which have been combined to produce the equivalent of a single 32-minute exposure. 

 

The images were obtained by the High Resolution Channel of the Advanced Camera for Surveys on the telescope. An occulting mask was placed in front of Neptune to reduce the planet's glare. In the image, a color composite of Neptune, taken one month earlier, has been inserted for context.

(1)  Naiad is the encircled point of light just to the left of Neptune.  

[download pdf / jpg ]

(2)  The orbits of all seven inner moons are indicated by blue lines. The next moon, Triton, is much further out and much larger than any of these small objects, which range from 20 km to 400 km in diameter. [download pdf /jpg]

(3)  This version of the image identifies all of the bodies visible in the image. Note that even the newly-discovered moon, provisionally identified as S/2004 N 1, is visible here as a faint dot. Only the third moon from the center--Despina--is not shown, because it was positioned behind the occulting mask, along with Neptune, at the time the images were taken. [download pdf/jpg ]

Neptune's slender rings are seen with remarkable clarity in this composite image taken by the Hubble Space Telescope. The rings were first imaged by the Voyager 2 spacecraft in 1989. Hubble obtained this image of Neptune in December, 2004, but astronomers only recently developed the image processing techniques needed to suppress the planet's intense glare and make this view possible. This image is composed of 26 individual exposures, which have been combined to produce the equivalent of a single 95-minute exposure. [download pdf/jpg ]

The outer ring, Adams, shows two distinct bright segments or "arcs" to the right of Neptune. At the time of the Voyager flyby, this ring contained four arcs, but two of them subsequently faded away. The arcs are believed to be confined by the gravitational influence of a nearby moon, Galatea, but the scientists do not currently understand why only two of the four arcs have survived for the intervening 15 years. An inner ring, Leverrier, is also visible.[downloadpdf/jpg ]

The images were obtained by the High Resolution Channel of the Advanced Camera for Surveys on the telescope. An occulting mask was placed in front of Neptune to reduce the planet's glare. In the image, a color composite of Neptune, taken one month earlier, has been inserted for context. [download pdf/jpg ]

Download the Press Conference Slides

Neptune’s tiny, innermost moon, Naiad, has now been seen for the first time since it was discovered by Voyager’s cameras in 1989. Dr. Mark Showalter, a senior research scientist at the SETI Institute in Mountain View, California, announced the result today in Denver, Colorado, at the annual meeting of the Division for Planetary Sciences of the American Astronomical Society. He and collaborators Dr. Jack Lissauer of the NASA Ames Research Center, Dr. Imke de Pater of UC Berkeley, and Robert French of the SETI Institute, also released a dramatic new image of Neptune’s puzzling rings and ring-arcs, which were first imaged by Voyager.

Naiad has been an elusive target ever since Voyager left the Neptune system,” said Dr. Showalter. From Earth, Neptune is 2 million times brighter than Naiad, andthetwo are separated by only one arcsecond. “This is equivalent to the width of a human hair from 50 feet away,” noted collaborator Lissauer. The team of astronomers needed to develop new techniques to suppress Neptune’s glare. Naiad was finally revealed, moving across a sequence of eight images taken during December 2004.

Strangely, Naiad appears to have veered significantly off course. The astronomers are puzzled by the fact that Naiad is now far ahead of its predicted orbital position. They wonder whether gravitational interactions with one of Neptune’s other moons may have caused it to speed up, although the details remain mysterious. Further observations will be needed in order to understand Naiad’s motion.

In addition to its moons, Neptune hosts a family faint rings and ring-arcs. The arcs have been changing slowly in the years since their discovery. Whereas Voyager saw a set of four closely-spaced arcs, the leading two arcs have been fading away, and are completely absent from the newest images. The trailing arcs, however, are essentially unchanged. This system of arcs is probably confined by the gravitational effects of the nearby moon Galatea, but the reason for the long-term changes is unknown. Dr. de Pater has also been following the ongoing evolution of the arcs from the 10-meter W. M. Keck telescope in Hawaii.

Showalter and his collaborators had previously announced the discovery of a tiny moon of Neptune in July. That moon, which is no more than 20 km (12 miles) across, goes by the provisional designation “S/2004 N 1”. The new results reported today are based on further analysis of the same images, which were all obtained by Hubble between 2004 and 2009. Although 100-km Naiad is much larger than the moon announced in July, it orbits much closer to Neptune and so has proven to be much harder to detect.

“It is always exciting to find new results in old data," Showalter remarked. "We keep discovering new ways to push the limit of what information can be gleaned from Hubble's vast collection of planetary images.”

Support for this work was provided by NASA through grant number from the SPACE TELESCOPE SCIENCE INSTITUTE, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555.

 

Contact Information

Media Contact:

Karen Randall
krandall@seti.org
(650) 960-4537

Science Contacts:

Mark Showalter
mshowalter@seti.org
650-810-0234 (office)
650-346-5276 (cell).

Jack Lissauer
Jack.J.Lissauer@nasa.gov.

Imke de Pater
imke@berkeley.edu.

Robert French
rfrench@seti.org.

About SETI  Institute

The mission of the SETI Institute is to explore, understand and explain the origin, nature and prevalence of life in the universe. The SETI Institute is a private, nonprofit organization dedicated to scientific research, education and public outreach. Founded in November 1984, the SETI Institute began operations on February 1, 1985. Today it employs over 120 scientists, educators and support staff. Research at the Institute is anchored by three centers. Gerry Harp is Director of the Center for SETI Research (Jill Tarter continues as Bernard M. Oliver Chair for SETI). David Morrison is the Director for the Carl Sagan Center for the Study of Life in the Universe. Edna DeVore leads our Center for Education and Public Outreach.
Online at http://www.seti.org